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Protostellar accretion traced with chemistry: Comparing synthetic C18O maps of embedded protostars to real observations
Søren Frimann, Jes K. Jørgensen, Paolo Padoan +1
Context: Understanding how protostars accrete their mass is a central question of star formation. One aspect of this is trying to understand whether the time evolution of accretion…
Supernova Driving. II. Compressive Ratio in Molecular-Cloud Turbulence
Liubin Pan, Paolo Padoan, Troels Haugbolle +1
The compressibility of molecular cloud (MC) turbulence plays a crucial role in star formation models, because it controls the amplitude and distribution of density fluctuations. Th…
Supernova Driving. I. The Origin of Molecular Cloud Turbulence
Paolo Padoan, Liubin Pan, Troels Haugboelle +1
Turbulence is ubiquitous in molecular clouds (MCs), but its origin is still unclear because MCs are usually assumed to live longer than the turbulence dissipation time. Interstella…
The relative and absolute ages of old globular clusters in the LCDM framework
Michele Trenti, Paolo Padoan, Raul Jimenez
Old Globular Clusters (GCs) in the Milky Way have ages of about 13 Gyr, placing their formation time in the reionization epoch. We propose a novel scenario for the formation of the…